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Far-infrared astronomy

From Wikipedia, the free encyclopedia

Far infrared image of the Andromeda galaxy from the Herschel Space Observatory

Far-infrared astronomy is the branch of astronomy and astrophysics that deals with objects visible in far-infrared radiation (extending from 30 μm towards submillimeter wavelengths around 450 μm).[1]

In the far-infrared, stars are not especially bright, but emission from very cold matter (140 Kelvin or less) can be observed that is not seen at shorter wavelengths. This is due to thermal radiation of interstellar dust contained in molecular clouds.[2]

These emissions are from dust in circumstellar envelopes around numerous old red giant stars. The Bolocam Galactic Plane Survey mapped the galaxy for the first time in the far-infrared.[2]

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  • NASA | Exploring Energy: Infrared
  • Infrared: Beyond the Visible
  • How do astronomers use infrared light to explore our Universe?

Transcription

Music Rob: Any form of matter that we can think of having a temperature, no matter how hot or cold, gives off thermal energy. [ Music ] Rob: A chair, a book, food, me. [ Music ] Rob: Everything around us, even the Earth itself, radiates thermal energy. Thermal energy forms the primary source of what we call infrared radiation. Infrared being the section of the electromagnetic spectrum that is just beyond visible light in terms of wavelength size. We cannot see infrared radiation. In fact, humans can only see a very small portion of the electromagnetic spectrum, but technology allows to detect and image matter in this very important part of the spectrum. NASA, NOAA, and other agencies, use thermal infrared imagery to study Earth systems in a way beyond what we could ever see. Through infrared data, we can study ocean and ice changes, map deforestation and forest fires, and monitor soil moisture and detect diseased vegetation. In fact, nearly every time we look at a weather report, from a heat wave to a hurricane, we are using thermal infrared imagery. Satellites detect infrared energy in a way that lets us study the Earth's weather patterns over both day and night, which is crucial for predicting the weather to come. In a way, it's as if the whole planet becomes visible to us at any time of day. Just over 200 years ago, Sir William Herschel discovered the existence of infrared by studying the sunlight passing through a simple prism. The prism separated all the colors that make up sunlight in an array called a spectrum. [ Music ] Here's a simple classroom activity that lets us see the phenomenon Herschel first observed. Herschel measured the temperatures of the different colors and found that the temperatures increased as he measured from violet to red. But what really struck him was the observation just beyond the visible spectrum. First, measure the ambient temperature of the box by placing the thermometers in the shade. Once the prism is adjusted for the widest spectrum possible, place the thermometers in the blue, yellow, and in the area just beyond red. Measuring over time, we will see the temperatures increase as we approach this infrared section of the spectrum. It may seem like a big jump to go from a prism on a box to the advanced imagery satellites provide around the globe, but it all helps to explain how there is more to light and energy than meets the eye. Music.

Telescopes

On 22 January 2014, European Space Agency scientists reported the detection, for the first definitive time, of water vapor on the dwarf planet, Ceres, largest object in the asteroid belt.[3] The detection was made by using the far-infrared abilities of the Herschel Space Observatory.[4] The finding is unexpected because comets, not asteroids, are typically considered to "sprout jets and plumes". According to one of the scientists, "The lines are becoming more and more blurred between comets and asteroids."[4]

Herschel Space Observatory

The Earth's atmosphere is opaque over most of the far-infrared, so most far-infrared astronomy is performed by satellites such as the Herschel Space Observatory,[5] Spitzer Space Telescope, IRAS, and Infrared Space Observatory. Upper-atmosphere observations are also possible, as conducted by the airborne SOFIA telescope.

Ground-based observations are limited to submillimetre wavelengths using high-altitude telescopes such as the James Clerk Maxwell Telescope, the Caltech Submillimeter Observatory, the High Elevation Antarctic Terahertz Telescope and the Submillimeter Array.

See also

References

  1. ^ A. Mampaso; M. Prieto; F. Sánchez (2003). Infrared Astronomy. Cambridge University Press. pp. 189–. ISBN 978-0-521-54810-6.
  2. ^ a b "Near, Mid and Far-Infrared". Caltech Infrared Processing and Analysis Center. Archived from the original on 2012-05-29. Retrieved 2013-01-28.
  3. ^ Küppers, Michael; O’Rourke, Laurence; Bockelée-Morvan, Dominique; Zakharov, Vladimir; Lee, Seungwon; von Allmen, Paul; Carry, Benoît; Teyssier, David; Marston, Anthony; Müller, Thomas; Crovisier, Jacques; Barucci, M. Antonietta; Moreno, Raphael (2014). "Localized sources of water vapour on the dwarf planet (1) Ceres". Nature. 505 (7484): 525–527. Bibcode:2014Natur.505..525K. doi:10.1038/nature12918. ISSN 0028-0836. PMID 24451541. S2CID 4448395.
  4. ^ a b Harrington, J.D. (22 January 2014). "Herschel Telescope Detects Water on Dwarf Planet - Release 14-021". NASA. Retrieved 22 January 2014.
  5. ^ Pilbratt, G. L.; Riedinger, J. R.; Passvogel, T.; Crone, G.; Doyle, D.; Gageur, U.; Heras, A. M.; Jewell, C.; Metcalfe, L.; Ott, S.; Schmidt, M. (2010). "HerschelSpace Observatory". Astronomy and Astrophysics. 518: L1. arXiv:1005.5331. Bibcode:2010A&A...518L...1P. doi:10.1051/0004-6361/201014759. ISSN 0004-6361. S2CID 118533433.
This page was last edited on 17 September 2023, at 11:10
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